1994
DOI: 10.1016/1350-4487(94)90086-8
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Cosmic ray contributions to dose rates for luminescence and ESR dating: Large depths and long-term time variations

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Cited by 3,169 publications
(1,615 citation statements)
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“…The selection of the average water content for age calculation was based on the depth and location of the sample relative to the expected groundwater level. The environmental dose rate was determined by gamma spectrometry (Murray et al, 1987) and by calculating the contribution from cosmic radiation according to Prescott and Hutton (1994). OSL measurements were done on large (8 mm) and small (2 mm) aliquots of 180-250 µm quartz grains with Risø TL/OSL readers equipped with 90 Sr/ 90 Y beta radiation sources (dose rate 0.10-0.33 Gy/s), blue (470 ± 30 nm; ~50 mW/cm 2 ) light sources, and detection was through a 7 mm U340 glass filter.…”
Section: Luminescence Datingmentioning
confidence: 99%
“…The selection of the average water content for age calculation was based on the depth and location of the sample relative to the expected groundwater level. The environmental dose rate was determined by gamma spectrometry (Murray et al, 1987) and by calculating the contribution from cosmic radiation according to Prescott and Hutton (1994). OSL measurements were done on large (8 mm) and small (2 mm) aliquots of 180-250 µm quartz grains with Risø TL/OSL readers equipped with 90 Sr/ 90 Y beta radiation sources (dose rate 0.10-0.33 Gy/s), blue (470 ± 30 nm; ~50 mW/cm 2 ) light sources, and detection was through a 7 mm U340 glass filter.…”
Section: Luminescence Datingmentioning
confidence: 99%
“…Water contents of the loess and fluvial sand samples were estimated to be 10 ± 2% and 5 ± 4% respectively, based on the field-measurement results. Cosmic-ray dose rate was calculated following Prescott and Hutton (1994).…”
Section: Appendix C: Details Of the Samples And Summary Of Dosimetrymentioning
confidence: 99%
“…8). Prescott and Hutton (1994), conversion factors of Guerin et al (2011), beta attenuation factors of Brennan (2003); internal K-content of 12.5 ± 0.5% (Huntley and Baril, 1997) 1.8 Q 9 47/61 2.80 ± 0.14 9.97 ± 0.63 1.33 ± 0.05 2.72 ± 0.32 13 ± 0.6 17 57.9 ± 3.1 21.3 ± 2.1 C-L2897 2.3 Q 9 48/61 2.85 ± 0.15 9.78 ± 0.57 1.36 ± 0.05 2.75 ± 0.32 10 ± 0.4 12 63.1 ± 3.3 23.0 ± 2.3 C-L2924 5.7 Q 11 32/42 2.55 ± 0.13 9.11 ± 0.53 1.39 ± 0.05 2.63 ± 0.30 20 ± 1.1 22 50.3 ± 3.1 19.1 ± 2.0 C-L2925 7.4 Q 11 41/60 2.80 ± 0.14 9.61 ± 0.55 1.37 ± 0.05 2.69 ± 0.28 28 ± 1.7 32 60.8 ± 4.1 22.6 ± 2.4 C-L2898 8.6 Q 15 35/69 2.64 ± 0.14 9.02 ± 0.53 1.37 ± 0.05 2.57 ± 0.32 26 ± 1.6 27 70.4 ± 4.7 27.3 ± 2.9 C-L2899 12.3 Q 14 37/61 2.49 ± 0.13 8.42 ± 0.49 1.22 ± 0.05 2.29 ± 0.27 38 ± 2.7 41 70.9 ± 5.7 30.9 ± 3.6 C-L2899 12.3 KF 14 25/26 2.49 ± 0.13 8.42 ± 0.49 1.22 ± 0.05 2.51 ± 0.30 25 ± 1.7 29 140.8 ± 9.9 56.0 ± 3.9 C-L2900 15.7 Q 18 36/60 2.63 ± 0.14 9.97 ± 0.58 1.52 ± 0.06 2.73 ± 0.29 30 ± 2.1 31 91.3 ± 6.6 33.4 ± 3.6 C-L2900 15.7 KF 18 28/28 2.63 ± 0.14 9.97 ± 0.58 1.52 ± 0.06 2.79 ± 0.31 20 ± 1.2 27 153.9 ± 9.7 55.2 ± 3.5 C-L2900 15.7 KF 18 23/28 2.63 ± 0.14 9.97 ± 0.58 1.52 ± 0.06 2.79 ± 0.31 13 ± 0.8 14 144.8 ± 8.3 51.9 ± 3.0* C-L2929 18.5 Q 20 38/53 2.65 ± 0.13 9.13 ± 0.52 1.39 ± 0.05 2.56 ± 0.27 22 ± 1.4 26 159.6 ± 10.1 62.4 ± 6.5 C-L2930 20.8 Q 17 33/54 2.87 ± 0.14 10.92 ± 0.62 1.84 ± 0.07 2.96 ± 0.35 41 ± 3.4 42 201.3 ± 18.0 67.9 ± 8.0…”
Section: (A) (B)mentioning
confidence: 99%
“…For K-feldspars, an internal potassium content of 12.5 ± 0.5% (Huntley and Baril, 1997) was assumed. The cosmic dose rate was calculated after Prescott and Hutton (1994).…”
Section: Luminescence Datingmentioning
confidence: 99%